From the 11 of 402 papers with an AI index.
76 citations
- Université Paris-SaclayFR139 papers
- Centre National de la Recherche ScientifiqueFR136 papers
- Sorbonne UniversitéFR131 papers
- University of BonnDE127 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT126 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT118 papers
- University of CambridgeGB118 papers
- University of OxfordGB117 papers
- Aix-Marseille UniversitéFR116 papers
- University of EdinburghGB115 papers
- Max Planck Institute for AstronomyDE114 papers
- Université Paris CitéFR111 papers
16 papers · 1 filter
Dynamical analysis of the 5:1 mean-motion resonance of the HD 202206 system
Yingyi Cao, Man Hoi Lee, Sabine Reffert +2
The HD 202206 system, which features two substellar companions with a 5:1 period ratio around a solar-type star, offers a rare opportunity to study high-order mean-motion resonance…
ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791
Georgina Dransfield, Antoine C. Petit, Amaury H. M. J. Triaud +45
Gas giant planets with periods orbiting Sun-like stars are a relatively uncommon outcome of planetary formation, and key questions about the nature and form…
Constraining an exoplanets magnetic field using star-planet interactions
D. Revilla, P. J. Amado, R. Luque +17
Theory predicts that a planet with a sufficiently strong magnetic field orbiting close to its host star could induce star-planet magnetic interactions. This is potentially observab…
A distant brown dwarf coplanar to a warm Jupiter and a hot super-Earth
MatÃas I. Jones, Luca Naponiello, Trifon Trifonov +21
In transiting planetary systems, in which planetary sizes are accurately determined from transit observations, the presence of transit-timing variations (TTVs), especially when com…
Atmospheric asymmetries in WASP-121 b revealed by rotational transits detected with JWST
Cyril Gapp, Aurélien Falco, Thomas M. Evans-Soma +6
Close-in exoplanets are tidally locked to their host star and thus exhibit extreme atmospheric temperature gradients. It has been theorized that the fraction of star light absorbed…
The Influence of the Fractal Dimension on Dust Evolution in Protoplanetary Disks
J. E. Schöll, C. P. Dullemond, C. Dominik
Context: During the first stages of dust coagulation in protoplanetary disks, the dust aggregates are expected to have a high degree of porosity. Most models of dust growth, howeve…